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Do lines of a particular element appear at the same wavelength in both emission and absorption line spectra?

No, lines of a particular element do not appear at the same wavelength in both emission and absorption line spectra. In absorption spectra, dark lines are seen where specific wavelengths are absorbed by elements in a cooler outer layer of a star or a cooler interstellar cloud. In contrast, emission spectra display bright lines when elements emit specific wavelengths of light at higher energy levels.


How would the spectra from galaxies appear?

They have broad emission lines of highly ionized elements.


Why do atomic spectra show individual lines instead of continuous spectra?

Atomic spectra show individual lines instead of continuous spectra because each line corresponds to a specific energy level transition of electrons within the atom. When electrons move between energy levels, they emit or absorb energy in the form of light at specific wavelengths, creating distinct spectral lines. This results in the observed pattern of individual lines in atomic spectra.


What causes spectra lines?

Absorption of energy at atom energy levels cause the line spectrum.


What is meant by the statement spectra lines are the fingerprints of elements?

Spectra lines are specific wavelengths of light emitted or absorbed by elements. Each element has a unique set of spectral lines, which allows scientists to identify elements present in a sample by comparing the observed spectra to known patterns, similar to how fingerprints are unique to individuals.


What are the differences between line spectra and continuous spectra in terms of their characteristics and properties?

Line spectra are composed of distinct, discrete lines of light at specific wavelengths, while continuous spectra consist of a continuous range of wavelengths without distinct lines. Line spectra are produced by excited atoms emitting light at specific energy levels, while continuous spectra are emitted by hot, dense objects like stars. Line spectra are unique to each element and can be used to identify elements, while continuous spectra are characteristic of hot, dense objects emitting thermal radiation.


Are emission lines spectra considered fingerprints of elements?

Yes, emission lines spectra are considered fingerprints of elements because each element emits light at specific wavelengths unique to that element. By analyzing the pattern of emission lines in a spectrum, scientists can identify the elements present in a sample.


What causes specific lines to appear in a line spectrum?

There are a couple of things that cause specific lines to appear in a line spectrum. Two of these things are density and wavelength.


Why do the emission spectra for hydrogen and helium differ?

The emission spectra for hydrogen and helium differ because each element has a unique arrangement of electrons in their atoms. This arrangement causes them to emit different wavelengths of light when excited, resulting in distinct spectral lines.


Why do we say atomic spectra are like fingerprints of the elements?

Atomic spectra are like fingerprints of elements because each element has a unique set of discreet emission or absorption lines in its spectrum. These lines correspond to specific energy levels of electrons within the atoms of that element. By analyzing the pattern and position of these lines in a spectrum, scientists can identify the elements present in a sample.


what automatic feature causes red and green lines to appear under words as you type?

AutoCorrect feature.


Why do stellar spectra have absorption lines?

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